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Table 4.

Fraction of outliers in the TOA datasets.

Pulsar 1D F8 2D 1D fscrunch
J0023+0923 53.8% 5.3% 3.8%
J0610−2100 9.1% 2.1% 1.1%
J0636+5128 12.2% 3.4% 1.5%
J1124−3653 82.1% 60.3% 56.3%
J1513−2550 18.8% 5.4% 6.8%
J1544+4937 34.8% 2.9% 2.6%
J1555−2908 13.9% 6.4% 6.4%
J1705−1903 0.6% 0.0% 0.0%
J1719−1438 68.8% 2.0% 1.0%
J1731−1847 41.4% 28.1% 77.4%
J1745+1017 16.4% 1.2% 2.4%
J1959+2048 43.4% 6.6% 8.9%
J2051−0827 9.0% 3.1% 3.4%
J2055+3829 17.4% 11.5% 11.7%
J2115+5448 36.2% 23.5% 40.4%
J2214+3000 90.2% 5.3% 4.0%
J2234+0944 14.4% 6.5% 6.4%
J2256−1024 48.2% 5.4% 5.1%

Notes. For each pulsars we compared TOAs extracted from eight frequency sub-bands of 64 MHz each using the standard template-matching method (“1D F8”), and TOAs extracted using the entire available bandwidth, with the wideband template-matching technique as implemented in the PulsePortraiture library (“2D”). For reference we also list the outlier rates as obtained when extracting TOAs from fully frequency-scrunched observations (“1D fscrunch”). Outliers are defined here are those with residuals larger than 1% of Pspin considering the uncertainty.

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